Fig. B.2
Distribution of 1 + δ in two cosmological boxes at z = 0.75. In both simulations, galaxies evolve according to De Lucia & Blaizot (2007) prescriptions. The cosmological parameters used as input are not the same, since taken from WMAP1 (red histogram) or WMAP3 (blue histogram). In this case, since we are not restricted to projected coordinates, we evaluated the density contrast using the 5NN in 3D space.
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